中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The Photometric Study of EX Dra: A Dwarf Nova Exhibiting a Titled and Precessional Disk

文献类型:期刊论文

作者Liu W(刘伟)2,3,4,5,6; Qian, Sheng-Bang4,5; Shi XD(施相东)2,3; Sun QB(孙起斌)2,3; Fang, Xiao-Hui1; Wang, Qi-Shan1
刊名ASTROPHYSICAL JOURNAL
出版日期2024-10-01
卷号974期号:1
ISSN号0004-637X
DOI10.3847/1538-4357/ad6f97
产权排序第4完成单位
文献子类Article
英文摘要We present a photometric study of EX Dra, a dwarf nova that has been extensively observed by the Transiting Exoplanet Survey Satellite. The data reveal the occurrence of 20 complete outbursts, exhibiting several intriguing and rare characteristics. The light curves exhibit a distinct superorbital signal with a period of approximately P sor similar to 4.39(7) days, along with a negative superhump showing an approximate period of P nsh similar to 4.805(1) hr, indicating that the accretion disk is tilted and undergoing precession with the period of P sor. In addition, the time-varying nature of P sor suggests that the precession period is fluctuating.The eclipsing light minima O - C analysis during quiescence shows an oscillation with period of 3.9(5) days, which is a little shorter than the superorbital period. We contend that this is unlikely to be a sudden alteration of the orbital period, but rather, it is influenced by the tilt and precession of the accretion disk. Notably, we found an amplitude shift in the outburst behavior from 3.5 mag with a periodicity of about 26 days to an amplitude of around 2.5 mag with a periodicity of about 12 days, which persisted for 14 yr before reverting. Furthermore, we have extracted quasiperiodic oscillations in the plateau at the noneclipsed phases, characterized by periods ranging between 37 and 40 minutes.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词QUASI-PERIODIC OSCILLATIONS ; KIC 9406652 ; CATACLYSMIC VARIABLES ; ACCRETION DISCS ; TILTED DISKS ; SUPERHUMPS ; INSTABILITIES ; SIMULATIONS ; MODEL
资助项目National Key R&D Program of China[2022YFE0116800]; National Natural Science Foundation of China[11933008]; National Natural Science Foundation of China[12103084]; Basic research project of Yunnan Province[202301AT070352]; Natural Science Foundation of Anhui Province[2208085QA23]; NASA Science Mission Directorate
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001329303300001
出版者IOP Publishing Ltd
资助机构National Key R&D Program of China[2022YFE0116800] ; National Natural Science Foundation of China[11933008, 12103084] ; Basic research project of Yunnan Province[202301AT070352] ; Natural Science Foundation of Anhui Province[2208085QA23] ; NASA Science Mission Directorate
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27638]  
专题云南天文台_双星与变星研究组
作者单位1.School of Mathematics, Physics and Finance, Anhui Polytechnic University, Wuhu 241000, People's Republic of China
2.University of Chinese Academy of Sciences, No. 1 Yanqihu East Rd., Huairou District, Beijing 101408, People's Republic of China;
3.Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, Kunming 650216, People's Republic of China;
4.Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, Kunming 650091, People's Republic of China;
5.Department of Astronomy, School of Physics and Astronomy, Yunnan University, Kunming 650091, People's Republic of China; qiansb@ynu.edu.cn;
6.College of Physics and Electronic Engineering, Xingtai University, Xingtai 054001, People's Republic of China;
推荐引用方式
GB/T 7714
Liu W,Qian, Sheng-Bang,Shi XD,et al. The Photometric Study of EX Dra: A Dwarf Nova Exhibiting a Titled and Precessional Disk[J]. ASTROPHYSICAL JOURNAL,2024,974(1).
APA 刘伟,Qian, Sheng-Bang,施相东,孙起斌,Fang, Xiao-Hui,&Wang, Qi-Shan.(2024).The Photometric Study of EX Dra: A Dwarf Nova Exhibiting a Titled and Precessional Disk.ASTROPHYSICAL JOURNAL,974(1).
MLA 刘伟,et al."The Photometric Study of EX Dra: A Dwarf Nova Exhibiting a Titled and Precessional Disk".ASTROPHYSICAL JOURNAL 974.1(2024).

入库方式: OAI收割

来源:云南天文台

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